activity
20062026
most citedThe Co-ordinated Radio and Infrared Survey for High Mass Star Formation (The CORNISH Survey) - I. Survey Design

183 citations · 1.3k across the 46 of their papers we have counts for

collaborators

46 papers

astro-ph.GA2026

The dynamical environment of the high-mass star-forming region G28.2880.364

Jyotirmoy Dey, Devendra K. Ojha, Jagadheep D. Pandian

Massive stars form within deeply embedded dust cores, and the development of hypercompact and ultracompact H II regions characterizes their early evolution. Identifying and analyzi…

astro-ph.GA2026

The 10-15 GHz radio continuum survey of the Galactic Plane with SKAO

A. Traficante, C. Mininni, F. Cavallaro +63

Star formation emerges from the complex interplay between gravity, turbulence, magnetic fields, and stellar feedback, all of which vary across spatial scales and Galactic environme…

astro-ph.GA2026

The Impact and Environment of Massive Stars and Stellar Clusters

Loren Anderson, Jagadheep D. Pandian, Jyotirmoy Dey +10

Massive stars and stellar clusters shape galactic evolution through powerful feedback mechanisms including radiation pressure, photoionization, stellar winds, and cosmic ray accele…

astro-ph.GA2026

Physical characterization and modeling of candidate Hyper-Compact HII Regions

I. T. Rodríguez-Esnard, S. Kurtz, J. D. Pandian +4

Hypercompact HII regions (HC) are regions of ionized gas associated with the early stages of high-mass star formation. With the aim of better understanding their characteristics, w…

astro-ph.GA2026

Detection of non-thermal radio emission components from the Orion Nebula: stellar jets, cloud collision or feedback from stellar winds?

Md Rashid, Nirupam Roy, Prasun Dutta +5

The Orion Nebula is the closest high-mass star-forming region, making it an ideal laboratory to investigate physical processes in complex star-forming environments. At radio freque…

astro-ph.GA2026★ 1 cited

Exploring the interplay between molecular and ionized gas in HII regions

S. Khan, A. M. Jacob, M. R. Rugel +8

We aim to constrain the kinetic temperature and H volume density of massive star-forming clumps associated with HII regions using multiple para-HCO transitions. In addition…